Splinter Meeting Relativistic

Relativistic astrophysics

Time: Thursday September 10, 16:15-18:00 and Friday September 11, 14:00-15:45 CEST (UTC+2)

Room: MW-2050

Convenor(s): Eva Hackmann, Odele Straub, Claus Lämmerzahl
University of Bremen and Excellence Cluster ORIGINS

This session covers the observational and theoretical aspects of the physics in strong gravitational fields and of the emergence of high energy phenomena. Strong gravity and relativity will be important for the formation and nature of white dwarfs, Neutron Stars and Black Holes. Physical phenomena in the vicinity of compact objects are lensing and shadows, the motion of stars in strong gravitational fields, gravitational waves, accretion disks, jets, and Gamma-Ray-Bursts. Also the aspects of relativity in cosmology and dark matter search will be part of this session.

Program

Thursday September 10, 16:15-18:00 Relativistic astrophysics (MW-2050)

16:15  Huanchen Hu:
New insights from the Double Pulsar

16:50  Dominik Schwarz:
Search for axion-like particles with strong gravitational lenses

17:25  Ke-Jung Chen:
Unveiling Magnetar-Powered Supernovae: From Superluminous to Broad-Line Type Ic

17:45  Navonil Saha:
Spin driven relativistic dynamics of supermassive black hole binaries in dense stellar environments

Friday September 11, 14:00-15:45 Relativistic astrophysics (MW-1050)

14:00  Vladimir Karas:
Particle acceleration by magnetized rotating black hole

14:30  Diego Calderón:
Establishing the role of relativistic precession on tidal disruption events

14:50  Ricard Aguilera Miret:
Magnetic disks around prompt-collapse black holes from binary neutron star mergers

15:10  Bhaskar Biswas:
Post-Merger Gravitational Waves as Probes of the Finite-Temperature Neutron Star Equation of State

15:30  Nikhita Vas:
Photon rings and shadows of Kerr black holes immersed in a swirling universe

Related contributions

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*) submitted abstracts, acceptance pending.